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Polarized proton projections Wolfram Fischer. 11 May 2012 RHIC Spin Collaboration Meeting BNL. Run-12 100 GeV polarized protons . Polarization (H-jet, i.e. intensity and time averaged) Blue 56 g 61.8% Yellow 57 g 56.6% (2009 g 2012). Run-12 255 GeV polarized protons .

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Polarized proton projections wolfram fischer

Polarized proton projectionsWolfram Fischer

11 May 2012

RHIC Spin Collaboration MeetingBNL


Run 12 100 gev polarized protons
Run-12 100 GeV polarized protons

Polarization (H-jet, i.e. intensity and time averaged)

Blue 56g61.8% Yellow 57g56.6% (2009g2012)

2


Run 12 255 gev polarized protons
Run-12 255 GeV polarized protons

Polarization (H-jet, i.e. intensity and time averaged)

Blue 48g50.3% Yellow 48g53.5% (2011g2012)

3


Rhic time in store
RHIC time-in-store

Low failure rates of all systems, even at raised energy.

4


Rhic polarized protons luminosity and polarization
RHIC polarized protons – luminosity and polarization

At 255 GeV in 2012

Lavg = 105x1030cm-2s-1

Pavg = 52%

Lavg +15% relative to 2011

Pavg+8% relative to 2011

FOM = LP2(single spin experiments)

FOM = LP4(double spin experiments)

5


New in run 12 run coordinator v schoeffer
New in Run-12 Run Coordinator: V. Schoeffer

  • 100 GeV

  • 2 new Landau cavities installed

  • Yellow primary collimator inspected (no sign of damage – concern for high intensity)

  • AGS horizontal alignment

  • 9 MHz system upgraded

  • AGS horizontal tune jump system timing improved

  • Operation from new MCR

  • Down ramps do not stop at park, park to injection 2x faster

  • 255 GeV

  • Increased store energy

  • Snake ramps between 100 GeV and 255 GeV

  • Scans of snake spin rotation axis angle and rotation angle

  • Test of longitudinal injection damper, Landau phase error compensation

  • Test of short AGS cycle

  • Test of Blue vertical phase shifter power supply (for electron lenses)

6


Polarization in run 12
Polarization in Run-12 Schoeffer

  • Difference between Blue and Yellow not understood(100 GeV PB > PY, 255 GeV PB <PY)

  • Expect only small further gains in ramp transmission

  • Polarization lifetime at store cannot be easily eliminated

  • Further P gains likely to come from source upgrade:larger initial polarization, and ability to reduce emittance

7


Preparation for run 13 pp
Preparation for Run-13 Schoefferpp

  • OPPIS upgrade

  • Electron lens installation

    • Also requires a new lattice (phase advance between IP8 and IP10 – phase shifters)

  • Polarimeter improvement

    • RF properties of pC polarimeter

    • Targets

  • RF

    • 9 MHz modification

    • Longitudinal injection damping

    • Landau phase compensation

8


Optically pumped polarized h source oppis a zelenski
Optically Pumped Polarized H Schoeffer– source (OPPIS) – A. Zelenski

Upgraded OPPIS (2013)

  • Goals:1. H− beam current increase to 10mA(order of magnitude)2. Polarization to 85-90%(~5% increase)

  • Upgrade components:

  • 1. Atomic hydrogen injector (collaboration with BINP Novosibirsk)

  • 2. Superconducting solenoid (3 T)

  • 3. Beam diagnostics and polarimetry

Source Neutralizer Ionizer Rb-cell Sona Na-jet (H+) (H0) (H+) (H0) (H−)

sc solenoid

10x intensity increase was demonstrated in a pulsed operation by using a very high-brightness Fast Atomic Beam Source instead of the ECR source

9


Oppis location 05 10 12
OPPIS location 05/10/12 Schoeffer

New Atomic Beam Source (ABS)

New superconducting solenoid

10


Rhic electron lenses motivation
RHIC electron lenses Schoeffer Motivation

Goal:

Compensate for 1 of 2 beam-beaminteractions with electron lenses

Then increase bunchintensity and luminosity (up to 2×)

Need with new polarized proton source − underconstruction, A. Zelenski

Bunch intensity in 2012 polarized proton physics store

bunches with 1 collision

bunches with 2 collisions

11


Rhic electron lenses compensation overview
RHIC electron lenses SchoefferCompensation overview

  • Basic idea:In addition to 2beam-beam collisions with positively charged beam have another collision with a negatively charged beam with the same amplitude dependence – and electron lens.

  • Exact compensation for:

  • short bunches

  • Dyx,y = kp between p-p and p-e collision

  • no nonlinearities between p-p and p-e

  • same amplitude dependent kick from p-p, p-e

  • only approximate realization possible

  • Deviations from ideal were extensively studied in simulations: Y. Luo et al. – accepted forpublication PRST-AB

FNAL - TEL

BNL - EBIS

Build on experience with Tevatron electron lenses V. Shiltsev, A. Burov, A. Valishev, G. Stancari, X.-L. Zhang, …

BNL Electron Beam Ion Source (EBIS)J. Alessi, E. Beebe, M. Okamura, A. Pikin, D. Raparia, …

12


Rhic electron lenses compensation overview1
RHIC electron lenses SchoefferCompensation overview

GS1 warm solenoidB = 0.8 T, I = 1200 A, P = 58 kW

SC main solenoid B = 6 T, I = 440 A+ 16 more magnets

CSB = GSB

GS2 warm solenoidB = 0.5 T, I = 730 A, P = 25 kW

CS2 = GS2

GSB warm solenoidB = 0.3 T, I = 770 A, P = 45 kW

CS1 = GS1

p

p

CSX/Y = GSX/Y

GSX/Y

Electron gunModes: DC, 100 Hz (setup), 80 kHz (1/turn)

Vmax = 10 kV, Imax = 1.5 A, P = 2×10-6 AV-3/2…Cathodes: LaB6 and IrCe (from Budker), 4.1 mm radius, Gaussian profile (2.8 s)

Electron collectorrP< 50 W/cm2, T < 125 °C

13


Electron lenses some hardware
Electron lenses some hardware

14



Luminosity projections for run 13
Luminosity projections for Run-13 some hardware

Polarization: 50-60% (depends largely on OPPIS progress)

Luminosity: electron lens commissioning, expect limited gains

16


Projections for p p
Projections for p some hardware⌃-p⌃

incremental changes

polarized source upgradeelectron lens commissioning

incremental changes(ex,y, es, DEstore, db/b…)

[Note: assume 12 weeks of physics, 8 weeks of ramp-up, start at ¼ of max]

17


Polarized proton projections summary
Polarized proton projections – summary some hardware

  • Have transformed Run-11 developments into operation in Run-12

  • Polarization

    • Further gains likely require source upgrade

    • Difference between Blue and Yellow not yet understood(both 100 GeV and 255 GeV)

  • Upgrades

    • OPPIS (expect gains in polarization and/or luminosity in Run-13)

    • Electron lenses (commissioning in Run-13, expect limited gains)

    • Longitudinal emittance

    • Polarimetry

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